DK Eyewitness - Astronomy
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Collenia<br />
Fossilized algae<br />
Dead plants and creatures buried in<br />
sediment are slowly turned to rock,<br />
becoming fossils. This rock contains the<br />
fossilized remains of tiny algae that<br />
were one of the earliest life forms.<br />
HUMAN DAMAGE<br />
Many scientists wonder if<br />
humans, like the dinosaurs, might<br />
also become extinct. The dinosaur<br />
seems to have been a passive victim<br />
of the changing Earth, while humans<br />
are playing a key role in the<br />
destruction of their environment.<br />
In the year 2000 there were more<br />
than 6 billion people on Earth—all<br />
producing waste and pollution. In<br />
addition to global warming that may<br />
be occurring due to the greenhouse<br />
effect, chemicals are being released<br />
that deplete the ozone layer—a layer<br />
in the atmosphere that keeps out<br />
dangerous ultraviolet radiation.<br />
Early life on earth<br />
The first life on Earth was primitive plants that took carbon<br />
dioxide from the air and released oxygen during photosynthesis.<br />
Animals evolved when there was enough oxygen in the<br />
atmosphere to sustain them. Knowledge about evolving life forms<br />
comes in the form of fossils in the rocks (left). However, life<br />
forms survive only if environmental conditions<br />
on Earth are suitable for them.<br />
The dinosaurs, for example,<br />
though perfectly adapted<br />
to their age, became<br />
extinct about 65<br />
million years ago.<br />
Plant-eating<br />
Edmontosaurus<br />
Life-giving atmosphere<br />
Our atmosphere extends out for about 600 miles (1,000 km).<br />
It sustains life and protects us from the harmful effects of solar<br />
radiation. It has several layers, but the life-sustaining layer is the<br />
troposphere, up to 6 miles (10 km) above Earth’s surface.<br />
4,500 mya<br />
Carbon<br />
dioxide<br />
Hydrogen<br />
Nitrogen<br />
Oxygen<br />
Today<br />
Magnetosphere<br />
shields Earth<br />
from solar wind<br />
Aurora<br />
Meteor shower<br />
(p.59)<br />
Weather satellite<br />
Ozone layer<br />
Maximum height<br />
for a balloon<br />
Maximum height<br />
for an airplane<br />
Mount Everest<br />
Troposphere<br />
Clouds<br />
Evolution of the atmosphere<br />
Since Earth was formed, the chemical<br />
makeup of the atmosphere has evolved.<br />
Carbon dioxide (CO ² ) decreased significantly<br />
between 4,500 and 3,000 million years<br />
ago (mya). There was a comparable rise in<br />
nitrogen. The levels of oxygen began to rise at<br />
the same time, due to photosynthesis<br />
of primitive plants, which used up<br />
CO ² and released oxygen.<br />
Facts about earth<br />
THE SPHERICAL EARTH<br />
As early as the 5th century bce<br />
the Greek philosophers<br />
had proposed that Earth is<br />
spherical, and by the 3rd<br />
century bce they had worked<br />
out a series of experiments to<br />
prove it. But it was not until the<br />
first satellites were launched<br />
in the late 1950s that humans<br />
saw what their planet looks<br />
like from space. The one<br />
feature that makes Earth<br />
unique is the great abundance<br />
of liquid water; more than twothirds<br />
of the surface is covered<br />
with water. Water makes Earth<br />
a dynamic place. Erosion, tides,<br />
weather patterns, and plentiful<br />
forms of life are all tied to the<br />
presence of water. There is more<br />
water in the Sahara Desert in North<br />
Africa than there is on Venus (pp.46–47).<br />
Oxygen/nitrogen<br />
atmosphere<br />
Solid iron core<br />
Molten iron core<br />
Rocky mantle<br />
Rocky crust<br />
• Sidereal period 365.26 days<br />
• Temperature –95°F to 130°F (–70°C to 55°C)<br />
• Rotational period 23 hr 56 min<br />
• Mean distance from the Sun 93 million miles/<br />
149.6 million km<br />
• Volume 1 • Mass 1<br />
• Density (water = 1) 5.52<br />
• Equatorial diameter 7,930 miles/12,760 km<br />
• Number of satellites 1 (the Moon)<br />
43